The 80th JSAP Autumn Meeting 2019

Presentation information

Oral presentation

2 Ionizing Radiation » 2.4 Accelerator Mass Spectrometry, Accelerator Beam Analysis

[21a-E303-1~12] 2.4 Accelerator Mass Spectrometry, Accelerator Beam Analysis

Sat. Sep 21, 2019 9:00 AM - 12:30 PM E303 (E303)

Masashi Ohno(Univ. of Tokyo), Masanori Kidera(Riken), Yasuto Miyake(Riken)

10:45 AM - 11:00 AM

[21a-E303-7] Distribution of the cosmogenic 10Be in the ocean.

Takeyasu Yamagata1,2, Hisao Nagai2, Hiroyuki Matsuzaki1, Hirofumi Tazoe3 (1.The Univ. of Tokyo, 2.Nihon Univ., 3.Hirosaki Univ.)

Keywords:Accelerator mass spectrometry, Cosmogenic nuclide, Ocean

It is necessary accumulation of oceanic Be-10 to assess Be-10 as a tracer for water mass. In this presentation, the north-south transection of Be-10 concentration shows in Indian Ocean during R/V Hakuho-maru in the KH09-5 cruise, and discuss a migration of Be-10.
According to hydrological data, Be-10 concentration in Antarctic intermediate water (AAIW) is relatively low concentration. The AAIW come from the low concentration surface water of the Antarctic Ocean. In deep-sea, the water mass, which named Common deep water, has high concentration. The Common deep water is originated from Atlantic deep sea, but the concentration of Be-10 in the Atlantic Ocean is lower than Common deep water. It is consider that the Be-10 in the surface Antarctic Ocean is transported down to the Antarctic deep sea by biogenic particles in Antarctic Ocean.